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Fine-Structure Constant
(redirected from Fine structure constant)

   Also found in: Wikipedia 0.01 sec.
fine-structure constant [′fīn ‚strək·chər ′kän·stənt]
(physics)
A fundamental dimensionless constant, equal toe2/(4πε0c) in International System (SI) units and toe2/(ℏc) in centimeter-gram-second (cgs) electrostatic units, whereeis the elementary charge, ℏ is Planck's constant divided by 2π,cis the speed of light, and ε0is the electric constant; numerically, it is equal to 0.007 297 352 533 ± 0.000 000 000 027 or to 1/(137.035 999 76 ± 0.000 000 50); symbolized α. Also known as Sommerfeld fine-structure constant.

Fine-Structure Constant 

(α), a dimensionless quantity formed from universal physical constants: α = e2/hc ≠ 1/137, where e is the elementary electric charge, h is Planck’s constant, and c is the speed of light in a vacuum. According to the most accurate measurements, which are based on the Josephson effect, α–1 = 137.0359 ± 0.0004. The constant α is called the fine-structure constant because it determines the fine structure of the energy levels of an atom in the sense that the magnitude of the fine-structure splitting is proportional to α2. In quantum electrodynamics, α is a natural parameter that characterizes the strength of the electromagnetic interaction.



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Adams simulated conditions in other universes by simultaneously varying three parameters: the gravitational constant, which determines the strength of gravity; the fine structure constant, which sets the strength of the electromagnetic force; and a number that determines the rate of nuclear reactions, which keep stars shining.
von Klitzing, Two-Dimensional Systems: A Method for the Determination of the Fine Structure Constant, Surf.
 
 
 
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